Psi5 Aurigae

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Psi5 Aurigae
Diagram showing star positions and boundaries of the Auriga constellation and its surroundings
Cercle rouge 100%.svg

The location of ψ5 Aurigae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension 06h 46m 44.3388s[1]
Declination +43° 34′ 38.737″[1]
Apparent magnitude (V) 5.25[2]
Characteristics
Spectral type G0 V[3]
U−B color index +0.06[2]
B−V color index +0.570[4]
Astrometry
Radial velocity (Rv) –24[5] km/s
Proper motion (μ) RA: –1.07[1] mas/yr
Dec.: +164.25[1] mas/yr
Parallax (π) 60.56 ± 0.73[1] mas
Distance 53.9 ± 0.6 ly
(16.5 ± 0.2 pc)
Absolute magnitude (MV) 4.13[5]
Details
Mass 1.079[6] M
Radius 1.18[6] R
Surface gravity (log g) 4.06[3] cgs
Temperature 5,989[3] K
Metallicity [Fe/H] +0.05[3] dex
Rotational velocity (v sin i) 5.03[4] km/s
Age 3.2[5] Gyr
Other designations
56 Aurigae, ADS 5425, BD+43°1595, FK5 255, HD 48682, HIP 32480, HR 2483, SAO 41330.[7]

Psi5 Aurigae5 Aur, ψ5 Aurigae) is the Bayer designation for a star[8] in the northern constellation of Auriga. It is faintly visible to the naked eye with an apparent visual magnitude of 5.25.[2] Based upon parallax measurements made during the Hipparcos mission, this star is approximately 53.9 light-years (16.5 parsecs) distant from Earth.[1] There is an optical companion[8] which is 36 arcseconds away and has an apparent magnitude of +8.4.

The spectrum of this star shows it to be a G-type main sequence star with a stellar classification of G0 V.[3] It is similar in size, mass,[6] and composition to the Sun,[3] making this a solar analog. It is radiating energy into space at an effective temperature of 5,989 K,[3] giving it the golden-hued glow of a G-type star.[9]

Observation in the infrared shows an excess emission that suggests the presence of a circumstellar disk of dust, known as a debris disk. This material has a mean temperature of 60 K, indicating that it is orbiting at a distance of about 29 astronomical units from the host star. The dust has about half the mass of the Moon and is around 600 million years old.[10] The star is being examined for evidence of extrasolar planets,[11] but none have been found so far.

References

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External links